The Astrophysical Journal · 1994 · 268 citations · 0 references
Natural SciencesAstronomyPhysicsAtmospheric ScienceInfrared AstronomySpectroscopyAtmospheric AbsorptionInterstellar GasMolecular CloudsAtmospheric Infrared AbsorptionInfrared Absorption LinesInfrared Absorption SpectraInfrared Absorption SpectroscopyInfrared SpectraMolecular Absorption FeaturesMolecular Cloud ObservationsVibrational Absorption Bands
Vibrational absorption by H2 and CO has been searched for toward infrared sources embedded in molecular clouds. H2 was detected toward NGC 2024 IRS 2 and possibly toward NGC 2264 (GL 989). CO was detected toward both sources. The results are consistent with the H2 ortho:para ratio being equilibrated at the cloud temperature. Toward NGC 2024, H2:CO = (3700<SUB>-2600</SUB><SUP>+3100</SUP>) (2 sigma limits), and toward NGC 2264, H2:CO less than 6000. Approximately one-third of all carbon is in gas-phase CO.